2018
DOI: 10.1140/epja/i2018-12516-4
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Semilocal momentum-space regularized chiral two-nucleon potentials up to fifth order

Abstract: We introduce new semilocal two-nucleon potentials up to fifth order in the chiral expansion. We employ a simple regularization approach for the pion-exchange contributions which (i) maintains the long-range part of the interaction, (ii) is implemented in momentum space and (iii) can be straightforwardly applied to regularize many-body forces and current operators. We discuss in detail the two-nucleon contact interactions at fourth order and demonstrate that three terms out of fifteen used in previous calculati… Show more

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Cited by 324 publications
(538 citation statements)
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“…Within χEFT, many studies have been carried out dealing with the construction and optimization of NN and 3N interactions [60,61,62,63,64,65,66,67,68,69,70,35,50,43,71,72,73,74,75,45,76,77,78,79,59,80,81,82,83] and accompanying isospin-symmetry-breaking corrections [84,85,86]. These interactions are typically formulated in momentum space, and include cutoff functions to regularize their behavior at large momenta.…”
Section: Nuclear Interactionsmentioning
confidence: 99%
“…Within χEFT, many studies have been carried out dealing with the construction and optimization of NN and 3N interactions [60,61,62,63,64,65,66,67,68,69,70,35,50,43,71,72,73,74,75,45,76,77,78,79,59,80,81,82,83] and accompanying isospin-symmetry-breaking corrections [84,85,86]. These interactions are typically formulated in momentum space, and include cutoff functions to regularize their behavior at large momenta.…”
Section: Nuclear Interactionsmentioning
confidence: 99%
“…where V is the bare NN interaction, the quantity ω is the so called starting energy. In the present work we consider spin unpolarized neutron matter, thus in equation (5) and in the following equations we drop the spin indices to simplify the mathematical notation. The Pauli operator | k a , k b Q k a , k b | projects on intermediate scattering states in which the momenta k a and k b of the two interacting neutrons are above their Fermi momentum k F since single particle states with momenta smaller that this value are occupied by the neutrons of the nuclear medium.…”
Section: Bethe-goldstone Equation [83]mentioning
confidence: 99%
“…Over the past twenty years, establishing this basic model of nuclear physics has undergone substantial progress, driven by two major factors. First, since the advent of chiral effective field theory (χEFT), originally proposed by Weinberg in the early 1990's [1,2], we can now systematically develop nuclear many-body interactions [3][4][5][6] and consistent electroweak currents [7][8][9][10][11][12][13] that are rooted in the fundamental symmetries exhibited by the underlying theory of Quantum Chromodynamics. Second, present computational resources allow to employ these interactions and current in sophisticated many-body methods to compute a variety of nuclear systems with controlled approximations [14][15][16][17][18][19][20].…”
Section: Introductionmentioning
confidence: 99%
“…Recently, accurate and precise chiral EFT potentials up to fifth order in the chiral expansion, i.e. N 4 LO, have been developed [73,74,75,76], and provide an extremely accurate description of NN data bases up to laboratory energies of 300 MeV with a χ 2 per datum close to one. These databases have been provided by the Nijmegen group [29,26], the VPI/GWU group [79], and more recently the Granada group [80,81,82].…”
Section: Chiral Effective Field Theorymentioning
confidence: 99%